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Fig. 3.

image

Inferred temperatures from NLTE IRIS and ALMA inversions. Temperature maps (in kK) at different optical depths from IRIS data alone (top left grouped panels) and with ALMA (bottom left grouped panels) corresponding to the synthetic data in Fig. 2. Rightmost panels: residuals in brightness temperature of the k core (top) and 1.25 mm (bottom) in the IRIS+ALMA fit. The error bars on the color maps indicate the median and the range between the 16th and 84th percentiles. The regions inside the dashed boxes are further investigated in Fig. 4.

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